Introducing General Relativity-Chapter 24

0.0(0)
studied byStudied by 0 people
0.0(0)
linked notesView linked note
full-widthCall with Kai
GameKnowt Play
New
learnLearn
examPractice Test
spaced repetitionSpaced Repetition
heart puzzleMatch
flashcardsFlashcards
Card Sorting

1/9

flashcard set

Earn XP

Description and Tags

These flashcards cover key concepts related to general relativity, including definitions of relevant astrophysical phenomena and principles.

Study Analytics
Name
Mastery
Learn
Test
Matching
Spaced

No study sessions yet.

10 Terms

1
New cards

White dwarf

A stellar remnant composed mostly of electron-degenerate matter, typically the end stage of stars with a mass less than 8 solar masses.

2
New cards

Neutron star

An astronomical object created when a massive star undergoes gravitational collapse after a supernova, consisting mostly of tightly packed neutrons.

3
New cards

Black hole

An object with a gravitational pull so strong that nothing, not even light, can escape from it; formed from the remnants of massive stars.

4
New cards

General relativity

Einstein's theory of gravitation that describes gravity as the warping of spacetime caused by mass.

5
New cards

Principle of equivalence

Einstein's idea that local effects of gravity are indistinguishable from acceleration; experiencing weightlessness in a freely falling elevator.

6
New cards

Spacetime

A four-dimensional continuum combining the three dimensions of space with the dimension of time, illustrating how mass warps the universe.

7
New cards

Escape velocity

The minimum speed an object must reach to break free from a celestial body's gravitational pull without additional propulsion.

8
New cards

Gravitational redshift

The phenomenon where light escaping a gravitational field is shifted to longer wavelengths, indicating a slower frequency due to time dilation.

9
New cards

Deflection of light

The bending of light's path due to the curvature of spacetime around massive objects.

10
New cards

Singularity

A point in space where density becomes infinite, typically at the center of a black hole, challenging our understanding of physics.